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Oscillatory phenomena in a solar network region

Published online by Cambridge University Press:  01 September 2008

Georgia Tsiropoula
Affiliation:
Institute for Space Applications and Remote Sensing, National Observatory of Athens, Lofos Koufos, 15236 P. Penteli, Greece email: [email protected]; [email protected]
Kostas Tziotziou
Affiliation:
Institute for Space Applications and Remote Sensing, National Observatory of Athens, Lofos Koufos, 15236 P. Penteli, Greece email: [email protected]; [email protected]
Pavol Schwartz
Affiliation:
Academy of Sciences of the Czech Republic, Astronomical Institut, CZ-25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
Petr Heinzel
Affiliation:
Academy of Sciences of the Czech Republic, Astronomical Institut, CZ-25165 Ondřejov, Czech Republic email: [email protected]; [email protected]
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Abstract

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We examine oscillatory phenomena in a solar network region from multi-wavelength, observations obtained by the ground-based Dutch Open Telescope (DOT), and by instruments on the spacecraft Solar and Heliospheric Observatory (SoHO). The observations were obtained during a coordinated observing campaign on October 14, 2005. The temporal variations of the intensities and velocities in two distinct regions of the quiet Sun were investigated: one containing several dark mottles and the other several bright points defining the network boundaries (NB). The aim is to find similarities and/or differences in the oscillatory phenomena observed in these two regions and in different spectral lines formed from the chromosphere to the transition region, as well as propagation characteristics of waves.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

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